Simon Glover

[Simon Glover @astroscog]

@CosmicRami @sarahkendrew Here's the link you want: https://t.co/4QpWr292SO

[Simon Glover @astroscog]

@watsoncomedian Thanks! DM sent.

[Simon Glover @astroscog]

@CatieSlaughts Feel free to DM me if you have questions that the website doesn't cover

[Simon Glover @astroscog]

@CatieSlaughts IMPRS-HD for positions in Heidelberg (at the University as well as the Max Planck). Application deadline is November 10, for details see here https://t.co/PiWX6z8w6m

[Simon Glover @astroscog]

@MarkWatsonHouse Thank you so much for all of this, it's been great fun

[Simon Glover @astroscog]

@DrEOChapman That looks familiar... 😀

[Simon Glover @astroscog]

@AndrasGaspar We don't have 5.6 mu, but we do have 2, 3 and 3.6 mu, once the NIRCAM level 3 data becomes available in MAST.

[Simon Glover @astroscog]

@JonKelvey @gbrammer @MAST_News @janiceleeastro This is a treasury proposal with no proprietary period, so the data becomes available in MAST pretty much as soon as it's taken.

[Simon Glover @astroscog]

@JonKelvey @gbrammer @MAST_News Quick clarification: this isn't commissioning data, it's from Cycle 1 proposal 2107 (PI: @janiceleeastro)

[Simon Glover @astroscog]

@FILWD @powersoffour started developing yt during his PhD (https://t.co/o7DbrYDDNI)

[Simon Glover @astroscog]

@KarenLMasters @astronomolly Sarah Nickerson (who doesn't seem to be on twitter) has published some Sci Fi short stories.

[Simon Glover @astroscog]

@KarenLMasters For the Galactic Centre, there's also the recent MeerKAT image: https://t.co/2tOFVfTJo5

[Simon Glover @astroscog]

@astro_biscuit @TomHaworthAstro The other is by Sharda et al (https://t.co/V6bAVyrWZt). Bottom line: even in the Pop. III context, with weak turbulence, there's substantial run-to-run variation in the degree of fragmentation and the resulting protostellar mass function

[Simon Glover @astroscog]

@astro_biscuit @TomHaworthAstro In case you missed them, there are a couple of recent papers looking at a similar issue in the context of Pop. III star formation. One is by my former student Katharina Wollenberg (https://t.co/o91C2lXJXm)

[Simon Glover @astroscog]

.@alexanderpji: takeaways: 1) enriching stellar populations vary between UFDs; 2) abundance scatter constrains metal mixing in UFDs #FirstStarsVI

[Simon Glover @astroscog]

.@alexanderpji: r-process elements more homogeneous than s-process elements. #FirstStarsVI

[Simon Glover @astroscog]

.@alexanderpji: current simulations produce much larger scatter, but Juta will solve everything in his talk #FirstStarsVI

[Simon Glover @astroscog]

.@alexanderpji: measure of [Ba/H] in 17 stars. Measure dispersion in [Ba/H] of ~0.2 dex (+/- 0.1 dex). Attributable to inhomog. mixing? If so, simulations should produce this level of scatter. #FirstStarsVI

[Simon Glover @astroscog]

.@alexanderpji: use r-process galaxy Reticulum II to measure inhomog. metal mixing - can do this as we know all the r-proc. elems come from the same enriching event #FirstStarsVI